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astro-ph.SR2026
Magnetohydrodynamic coronal modelling with high-fidelity magnetograms
Haopeng Wang, Stefaan Poedts, Wensi Wang +16
To resolve coronal structures in detail, it is essential to constrain the coronal model using high-fidelity magnetograms with minimal smoothing. In this paper, we improve the numer…
astro-ph.SR2026
Supersonic flows observed by THEMIS related to a coronal bright point and filament
Garima Karki, Brigitte Schmieder, Ramesh Chandra +3
In this paper, we report on the dynamics of the fine structure of a solar quiescent filament observed on September 28, 2023, with the Télescope Héliographique pour l'Etude du Magné…